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arXiv · astro-ph/0404487

Quasar Variability Measurements With SDSS Repeated Imaging and POSS Data

Abstract

We analyze the properties of quasar variability using repeated SDSS imaging data in five UV-to-far red photometric bands, accurate to 0.02 mag, for 13,000 spectroscopically confirmed quasars. The observed time lags span the range from 3 hours to over 3 years, and constrain the quasar variability for rest-frame time lags of up to two years, and at rest-frame wavelengths from 1000 Ang. to 6000 Ang. We demonstrate that 66,000 SDSS measurements of magnitude differences can be described within the measurement noise by a simple function of only three free parameters. The addition of POSS data constrains the long-term behavior of quasar variability and provides evidence for a turn-over in the structure function. This turn-over indicates that the characteristic time scale for optical variability of quasars is of the order 1 year.

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BibTeXRIS

Z Ivezic, R. H. Lupton, M. Juric, S. Anderson, P. B. Hall, G. T. Richards, C. M. Rockosi, D. E. Vanden Berk, E. L. Turner, G. R. Knapp, J. E. Gunn, D. Schlegel, M. A. Strauss, D. P. Schneider. 2004-04-26. Quasar Variability Measurements With SDSS Repeated Imaging and POSS Data. https://doi.org/10.1017/s1743921304003126

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